Abstract
As hydrodynamic simulations increase in scale and resolution,
identifying structures with non-trivial geometries or regions of general
interest becomes increasingly challenging. There is a growing need for
algorithms that identify a variety of different features in a simulation
without requiring a `by eye' search. We present tensor classification as
such a technique for smoothed particle hydrodynamics (SPH). These
methods have already been used to great effect in N-Body cosmological
simulations, which require smoothing defined as an input free parameter.
We show that tensor classification successfully identifies a wide range
of structures in SPH density fields using its native smoothing, removing
a free parameter from the analysis and preventing the need for
tessellation of the density field, as required by some classification
algorithms. As examples, we show that tensor classification using the
tidal tensor and the velocity shear tensor successfully identifies
filaments, shells and sheet structures in giant molecular cloud
simulations, as well as spiral arms in discs. The relationship between
structures identified using different tensors illustrates how different
forces compete and co-operate to produce the observed density field. We
therefore advocate the use of multiple tensors to classify structure in
SPH simulations, to shed light on the interplay of multiple physical
processes.
| Original language | English |
|---|---|
| Pages (from-to) | 2501-2513 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 457 |
| Issue number | 3 |
| Early online date | 10 Feb 2016 |
| DOIs | |
| Publication status | Published - 11 Apr 2016 |
Keywords / Materials (for Non-textual outputs)
- methods: numerical
- stars: formation
- ISM: kinematics and dynamics